Structure of the Spiral Galaxy NGC 300
In 1963, Toomre built up classes of mass models for the highly flattened galaxies which have free parameters n, an and Cn. In order to keep the universal dimension, we adopt parameters bn(Cn2 = an2n+2*bn2/(n-1)!) instead of Cn. Series of the normalized Toomre's mass models (G = Vmax = Rmax = 1,...
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Korean Space Science Society (KSSS)
1992-06-01
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doaj-4830731e513e499ea163e839a19532ff2020-11-24T23:23:19ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14091992-06-01911129Structure of the Spiral Galaxy NGC 300Myung-Hyun Rhee0Mun-Suk Chun1Department of Astronomy and Atmospheric Science, Yonsei University, Seoul 120-749, KoreaDepartment of Astronomy and Atmospheric Science, Yonsei University, Seoul 120-749, KoreaIn 1963, Toomre built up classes of mass models for the highly flattened galaxies which have free parameters n, an and Cn. In order to keep the universal dimension, we adopt parameters bn(Cn2 = an2n+2*bn2/(n-1)!) instead of Cn. Series of the normalized Toomre's mass models (G = Vmax = Rmax = 1, n =1 to 7) are derived and the normalized parameters an and bn to an(=an*rmax) and bn(=bn*Vmax/rmax), we can get the generalization of Toomre's mass model.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_11.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Myung-Hyun Rhee Mun-Suk Chun |
spellingShingle |
Myung-Hyun Rhee Mun-Suk Chun Structure of the Spiral Galaxy NGC 300 Journal of Astronomy and Space Sciences |
author_facet |
Myung-Hyun Rhee Mun-Suk Chun |
author_sort |
Myung-Hyun Rhee |
title |
Structure of the Spiral Galaxy NGC 300 |
title_short |
Structure of the Spiral Galaxy NGC 300 |
title_full |
Structure of the Spiral Galaxy NGC 300 |
title_fullStr |
Structure of the Spiral Galaxy NGC 300 |
title_full_unstemmed |
Structure of the Spiral Galaxy NGC 300 |
title_sort |
structure of the spiral galaxy ngc 300 |
publisher |
Korean Space Science Society (KSSS) |
series |
Journal of Astronomy and Space Sciences |
issn |
2093-5587 2093-1409 |
publishDate |
1992-06-01 |
description |
In 1963, Toomre built up classes of mass models for the highly flattened galaxies which have free parameters n, an and Cn. In order to keep the universal dimension, we adopt parameters bn(Cn2 = an2n+2*bn2/(n-1)!) instead of Cn. Series of the normalized Toomre's mass models (G = Vmax = Rmax = 1, n =1 to 7) are derived and the normalized parameters an and bn to an(=an*rmax) and bn(=bn*Vmax/rmax), we can get the generalization of Toomre's mass model. |
url |
http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_11.pdf |
work_keys_str_mv |
AT myunghyunrhee structureofthespiralgalaxyngc300 AT munsukchun structureofthespiralgalaxyngc300 |
_version_ |
1725564112878960640 |